例文 | 共起表現 |
「λ」の共起表現一覧(1語右で並び替え)
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Introducing an undetermined multiplier | λ, a Lagrangian is constructed as |
and for | λ an infinite limit ordinal, |
the process (a, | λ).P can perform an action a at rate λ and continu |
If the (m+1)th order of | λ and (m)th order of (λ + Δλ) lie at the same angl |
ty, compact sets) K and L with probabilities 1 − | λ and λ respectively, then Vitale's random Brunn-M |
the following property: there exists a worldline | λ and an event p such that all events along λ are |
del with the critical point of j being κ, j(κ) ≥ | λ, and V(λ) is a subset of j(M). |
onformations, which are described by the symbols | λ and δ. |
he two groups are proportional with hazard ratio | λ and d1 and d2 are the probabilities that a subje |
ate, which can be resolved into two enantiomers ( | Λ and Δ) by the formation of the d-α-bromocamphor- |
In such a case we need a better first guess at | λ, and that may not be easy to get; the alternativ |
Lambda Andromedae ( | λ And, λ Andromedae) is a binary star in the const |
Lambda Aquilae ( | λ Aql, λ Aquilae) is a star in the constellation A |
Lambda Aquarii ( | λ Aqr, λ Aquarii) is a star in the constellation A |
where | λ are mean longitudes of the moons. |
The Lyapunov exponents, | λ are approximately 0.1981, 0, −0.6581 and the Kap |
rmula may fail to converge; this will occur when | λ as computed by the equation above is greater tha |
Lambda Aurigae ( | λ Aur, λ Aurigae) is a binary star in the constell |
Its companion, | λ Aurigae B, is 29 arcseconds away and has an appa |
o has two optical companions, the 12th magnitude | λ Aurigae C at 42 arcseconds and the magnitude +8. |
The primary component, | λ Aurigae A, is a yellow G-type subgiant with an a |
In particle physics, lambda ( | Λ) baryons are baryons containing an up quark, a d |
any two varieties occur together in exactly | λ blocks; |
of the particle p was related to its wavelength | λ by what is now known as the de Broglie relation |
nt of the group of quaternionic automorphisms of | Λ by the group ±1 of scalars. |
yle of obtaining the normal form of terms in the | λ calculus by appealing to their denotational sema |
oncept of "effective calculability" based on his | λ calculus and by Alan Turing in the same year wit |
λ Canis Majoris is a blue-white B-type main sequen | |
β Cassiopeiae, κ Cassiopeiae, η Cassiopeiae and | λ Cassiopeiae. |
Lambda Centauri ( | λ Cen, λ Centauri) is a star in the constellation |
λ Centauri is a blue-white B-type giant with an ap | |
This star, along with α Cet (Menkar), | λ Cet (Menkar), γ Cet (Kaffaljidhma), μ Cet, ξ1 Ce |
is star, along with γ Cet (Kaffaljidhma), δ Cet, | λ Cet (Menkar), μ Cet, ξ1 Cet and ξ2 Cet were Al K |
Cet as Al Kaff al Jidhmah IV (exclude α Cet and | λ Cet) |
Lambda Canis Majoris ( | λ CMa, λ Canis Majoris) is a star in the constella |
Aksys Games released | Λ Core Plus for the US market on April 7, 2009 for |
The apparent magnitude of | λ Crucis is 4.6, but it is not stable. |
λ Crucis is located at 360 light-years from the Su | |
Lambda Crucis ( | λ Crucis / λ Cru) is a star in the constellation C |
where | λ denotes Lebesgue measure and ρ is the backward s |
B. (1982), "Nucleotide sequence of bacteriophage | λ DNA", Journal of Molecular Biology 162 (4): 729- |
For example, a | λ DNA-HindIII Digest: a common lambda DNA ladder t |
tar association consisting this star, along with | λ Eri, ψ Eri and τ Ori |
y assigning the zero mass particles a small mass | λ, evaluating the corresponding expression and the |
Lambda Geminorum ( | λ Gem, λ Geminorum) is a Class A3, fourth-magnitud |
crystals, there is a minimum possible wavelength | λ, given by twice the equilibrium separation betwe |
With β, δ, θ. ι, and | λ Gru, it belonged to Piscis Austrinus in traditio |
of the (Southern) Fish: it, with α, δ, θ. ι, and | λ Gru, belonged to Piscis Austrinus in traditional |
node i carries, Ai,j is the adjacency matrix and | λ happens to be the principal eigenvalue (although |
where | Λ has a finite value that represents the fastest d |
eigenvector of Th with respect to the eigenvalue | λ, i.e. |
ss fin of the last record of the output list (or | Λ if that list is still empty). |
bedding j:(Vκ, ∈, P) → (Vλ, ∈, P) for some κ and | λ in S. |
behaviour (measured using the Lyapunov exponent | λ) in the a−b plane for a given periodic sequence |
attP and attB of | λ integrase, see lambda phage). |
If | Λ is a harmonious set and F is a finite set then t |
A set | Λ is harmonious if every weak character may be app |
If | λ is any ordinal, κ is λ-supercompact means that t |
Where D00 is the beam waist size, and | λ is the wavelength. |
successor operation S; in precise terms, we say | λ is a limit ordinal if and only if λ > 0 and for |
The value of the cosmological constant, | Λ, is ~2 x 10−35s−2. |
where | λ is the wavelength of the spectral peak of intere |
where | λ is the Marquardt parameter and I is an identity |
where | λ is the wavelength, f is the frequency, and c is |
Sometimes, a cosmological constant | Λ is included in the Lagrangian so that the new ac |
If | λ is any ordinal, κ is λ-strong means that κ is a |
e a is the period of the diffraction grating and | λ is the wavelength of the light incident on the g |
ength (distance from pinhole to image plane) and | λ is the wavelength of light. |
he radiator (or the diametre of the antenna) and | λ is the wavelength of the radio wave. |
into a transitive class M that includes Vλ where | λ is the first fixed point above the critical poin |
ope as , where d is the resolvable feature size, | λ is the wavelength of light, n is the index of re |
er model M with critical point κ and λM⊆M, where | λ is the supremum of jnκ for positive integers n. |
λ is the mean free path | |
Λ is a set of formal languages; | |
where | λ is the signal's wavelength. |
Phoenician letter gave rise to the Greek Lambda ( | Λ), Latin L, and Cyrillic El (Л). |
Since | λ lies in p's past, the Turing machine can signal |
Lambda Lyrae ( | λ Lyr) is a 5th magnitude star in the constellatio |
Color the point (a,b) according to the value of | λ obtained. |
Because only certain wavelengths ( | λ) of light are absorbed - those matching exactly |
A strong character is a restriction to | Λ of a continuous homomorphism from G to T, that i |
Lambda Ophiuchi ( | λ Oph, λ Ophiuchi) is a binary star system in the |
It is denoted with | λ or sometimes Λ or ε. |
λ Ori X-1 has visual designation HDE 245059. | |
The Orion X-ray source, | λ Ori X-1, is not in any Uhuru catalog. |
λ Ori X-1 is actually a discovery with the Einstei | |
λ Ori X-1 is spectral type K1, rotating at ~25 km/ | |
λ Ori is one of the youngest stars of the λ Ori as | |
Lambda Orionis ( | λ Ori, λ Orionis) is a star in the constellation O |
ena), but was somehow also mistakenly applied to | λ Orionis and the name stuck. |
ion of either a lytic or lysogenic life cycle in | λ phage - with high concentrations of cIII promoti |
S → | λ provided S does not appear on the right side of |
where | λ represents the gaugino field (a spinor) and Λ is |
λ Sco and υ Sco, two stars at the end of the scorp | |
Lambda Serpentis ( | λ Ser, λ Serpentis) is a star in the constellation |
Lambda Sagittarii ( | λ Sgr, λ Sagittarii) is a star within the constell |
(named for W. Hugh Woodin) is a cardinal number | λ such that for all functions |
Along with | λ Tau, it was one of the first stars on which rota |
Lambda Telescopii ( | λ Tel, λ Telescopii) is a star in the constellatio |
distributed random variable hain with parameter | λ, that is, with probability density function |
with n0 the refractive index of the solvent, | λ the wavelength of the light source, dn/dc the re |
Here Nx is the number of x atoms per volume, | λ the electron escape depth, θ the analyzer angle, |
th s the shear distance, df the fringe distance, | λ the wavelength and γ the angular deviation of th |
with a Poisson distribution with expected value | λ, then its nth moment is |
inal number κ is called η-extendible if for some | λ there is a nontrivial elementary embedding j of |
The World Is a Thorn (also stylized The World Is | Λ Thorn) is Demon Hunter's fifth studio album, whi |
rent precision electroweak measurements restrict | Λ to more than a few TeV. |
This causes the wavelength | λ to decrease, which means that the signal then tr |
he small quantum cohomology with coefficients in | Λ to be |
Lambda Ursae Majoris ( | λ UMa, λ Ursae Majoris) is a star in the constella |
ved into enantiomers that are described as Δ and | Λ. Usually the resolution entails use of tartrate s |
Lambda Velorum ( | λ Vel or λ Velorum) is a star in the constellation |
gen "fuel" much faster than do smaller stars and | λ Velorum is estimated to be only some 27 million |
Lambda Virginis ( | λ Vir, λ Virginis) is a binary star in the constel |
tements has cardinality below a certain cardinal | λ; we may then refer to λ-compactness. |
Compton recoil with momentum proportional to h / | λ, where h is Planck's constant. |
例文 | 共起表現 |
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